Powerflow

The power flow problem is about the calculation of voltage magnitudes and angles for one set of buses. The solution is obtained from a given set of voltage magnitudes and power levels for a specific model of the network configuration. The power flow solution exhibits the voltages and angles at all buses and real and reactive flows can be deduced from the same.

Power System Model

Power systems are modeled as a network of buses (nodes) and branches (lines). To a network bus, components such a generator, load, and transmission substation can be connected. Each bus in the network is fully described by the following four electrical quantities:

$\vert V_{k} \vert$ : the voltage magnitude
$\theta_{k}$ : the voltage phase angle
$P_{k}$ : the active power
$Q_{k}$ : the reactive power

There are three types of networks buses: VD bus, PV bus and PQ bus. Depending on the type of the bus, two of the four electrical quantities are specified as shown in the table below.

Bus Type	Known	Unknown
$VD$	$\vert V_{k} \vert, \theta_{k}$	$P_{k}, Q_{k}$
$PV$	$P_{k}, \vert V_{k} \vert$	$Q_{k}, \theta_{k}$
$PQ$	$P_{k}, Q_{k}$	$\vert V_{k} \vert, \theta_{k}$

Single Phase Power Flow Problem

The power flow problem can be expressed by the goal to bring a mismatch function $\vec{f}$ to zero. The value of the mismatch function depends on a solution vector $\vec{x}$ : $\vec{f}(\vec{x}) = 0$

As $\vec{f}(\vec{x})$ will be nonlinear, the equation system will be solved with Newton-Raphson:

$-\textbf{J}(\vec{x}) \Delta \vec{x} = \vec{f} (\vec{x})$

where $\Delta \vec{x}$ is the correction of the solution vector and $\textbf{J}(\vec{x})$ is the Jacobian matrix. The solution vector $\vec{x}$ represents the voltage $\vec{V}$ by polar or cartesian quantities. The mismatch function $\vec{f}$ will either represent the power mismatch $\Delta \vec{S}$ in terms of

$\left [ \begin{array}{c} \Delta \vec{P} \ \Delta \vec{Q} \end{array} \right ]$

or the current mismatch $\Delta \vec{I}$ in terms of

$\left [ \begin{array}{c} \Delta \vec{I_{real}} \ \Delta \vec{I_{imag}} \end{array} \right ]$

where the vectors split the complex quantities into real and imaginary parts. Futhermore, the solution vector $\vec{x}$ will represent $\vec{V}$ either by polar coordinates

$\left [ \begin{array}{c} \vec{\delta} \ \vert \vec{V} \vert \end{array} \right ]$

or rectangular coordinates

$\left [ \begin{array}{c} \vec{V_{real}} \ \vec{V_{imag}} \end{array} \right ]$

This results in four different formulations of the powerflow problem:

with power mismatch function and polar coordinates
with power mismatch function and rectangular coordinates
with current mismatch function and polar coordinates
with current mismatch function and rectangular coordinates

To solve the problem using NR, we need to formulate $\textbf{J} (\vec{x})$ and $\vec{f} (\vec{x})$ for each powerflow problem formulation.

Powerflow Problem with Power Mismatch Function and Polar Coordinates

Formulation of Mismatch Function

The injected power at a node $k$ is given by: $S_{k} = V_{k} I _{k}^{*}$

The current injection into any bus $k$ may be expressed as: $I_{k} = \sum_{j=1}^{N} Y_{kj} V_{j}$

Substitution yields:

\begin{align} S_{k} &= V_{k} \left ( \sum_{j=1}^{N} Y_{kj} V_{j} \right )^{*} \nonumber \\ &= V_{k} \sum_{j=1}^{N} Y_{kj}^{*} V_{j} ^{*} \nonumber \end{align}

We may define $G_{kj}$ and $B_{kj}$ as the real and imaginary parts of the admittance matrix element $Y_{kj}$ respectively, so that $Y_{kj} = G_{kj} + jB_{kj}$ . Then we may rewrite the last equation:

\begin{align} S_{k} &= V_{k} \sum_{j=1}^{N} Y_{kj}^{*} V_{j}^{*} \nonumber \\ &= \vert V_{k} \vert \angle \theta_{k} \sum_{j=1}^{N} (G_{kj} + jB_{kj})^{*} ( \vert V_{j} \vert \angle \theta_{j})^{*} \nonumber \\ &= \vert V_{k} \vert \angle \theta_{k} \sum_{j=1}^{N} (G_{kj} - jB_{kj}) ( \vert V_{j} \vert \angle - \theta_{j}) \nonumber \\ &= \sum_{j=1} ^{N} \vert V_{k} \vert \angle \theta_{k} ( \vert V_{j} \vert \angle - \theta_{j}) (G_{kj} - jB_{kj}) \nonumber \\ &= \sum_{j=1} ^{N} \left ( \vert V_{k} \vert \vert V_{j} \vert \angle (\theta_{k} - \theta_{j}) \right ) (G_{kj} - jB_{kj}) \nonumber \\ &= \sum_{j=1} ^{N} \vert V_{k} \vert \vert V_{j} \vert \left ( cos(\theta_{k} - \theta_{j}) + jsin(\theta_{k} - \theta_{j}) \right ) (G_{kj} - jB_{kj}) \end{align}

If we now perform the algebraic multiplication of the two terms inside the parentheses, and collect real and imaginary parts, and recall that $S_{k} = P_{k} + jQ_{k}$ , we can express (1) as two equations: one for the real part, $P_{k}$ , and one for the imaginary part, $Q_{k}$ , according to:

\begin{align} {P}_{k} = \sum_{j=1}^{N} \vert V_{k} \vert \vert V_{j} \vert \left ( G_{kj}cos(\theta_{k} - \theta_{j}) + B_{kj} sin(\theta_{k} - \theta_{j}) \right ) \\ {Q}_{k} = \sum_{j=1}^{N} \vert V_{k} \vert \vert V_{j} \vert \left ( G_{kj}sin(\theta_{k} - \theta_{j}) - B_{kj} cos(\theta_{k} - \theta_{j}) \right ) \end{align}

These equations are called the power flow equations, and they form the fundamental building block from which we solve the power flow problem.

We consider a power system network having $N$ buses. We assume one VD bus, $N_{PV}-1$ PV buses and $N-N_{PV}$ PQ buses. We assume that the VD bus is numbered bus $1$ , the PV buses are numbered $2,…,N_{PV}$ , and the PQ buses are numbered $N_{PV}+1,…,N$ . We define the vector of unknown as the composite vector of unknown angles $\vec{\theta}$ and voltage magnitudes $\vert \vec{V} \vert$ :

\begin{align} \vec{x} = \left[ \begin{array}{c} \vec{\theta} \\ \vert \vec{V} \vert \\ \end{array} \right ] = \left[ \begin{array}{c} \theta_{2} \\ \theta_{3} \\ \vdots \\ \theta_{N} \\ \vert V_{N_{PV+1}} \vert \\ \vert V_{N_{PV+2}} \vert \\ \vdots \\ \vert V_{N} \vert \end{array} \right] \end{align}

The right-hand sides of equations (2) and (3) depend on the elements of the unknown vector $\vec{x}$ . Expressing this dependency more explicitly, we rewrite these equations as:

\begin{align} P_{k} = P_{k} (\vec{x}) \Rightarrow P_{k}(\vec{x}) - P_{k} &= 0 \quad \quad k = 2,...,N \\ Q_{k} = Q_{k} (\vec{x}) \Rightarrow Q_{k} (\vec{x}) - Q_{k} &= 0 \quad \quad k = N_{PV}+1,...,N \end{align}

We now define the mismatch vector $\vec{f} (\vec{x})$ as:

\begin{align} \vec{f} (\vec{x}) = \left [ \begin{array}{c} f_{1}(\vec{x}) \\ \vdots \\ f_{N-1}(\vec{x}) \\ ------ \\ f_{N}(\vec{x}) \\ \vdots \\ f_{2N-N_{PV} -1}(\vec{x}) \end{array} \right ] = \left [ \begin{array}{c} P_{2}(\vec{x}) - P_{2} \\ \vdots \\ P_{N}(\vec{x}) - P_{N} \\ --------- \\ Q_{N_{PV}+1}(\vec{x}) - Q_{N_{PV}+1} \\ \vdots \\ Q_{N}(\vec{x}) - Q_{N} \end{array} \right] = \left [ \begin{array}{c} \Delta P_{2} \\ \vdots \\ \Delta P_{N} \\ ------ \\ \Delta Q_{N_{PV}+1} \\ \vdots \\ \Delta Q_{N} \end{array} \right ] = \vec{0} \end{align}

That is a system of nonlinear equations. This nonlinearity comes from the fact that $P_{k}$ and $Q_{k}$ have terms containing products of some of the unknowns and also terms containing trigonometric functions of some the unknowns.

Formulation of Jacobian

As discussed in the previous section, the power flow problem will be solved using the Newton-Raphson method. Here, the Jacobian matrix is obtained by taking all first-order partial derivates of the power mismatch functions with respect to the voltage angles $\theta_{k}$ and magnitudes $\vert V_{k} \vert$ as:

\begin{align} J_{jk}^{P \theta} &= \frac{\partial P_{j} (\vec{x} ) } {\partial \theta_{k}} = \vert V_{j} \vert \vert V_{k} \vert \left ( G_{jk} sin(\theta_{j} - \theta_{k}) - B_{jk} cos(\theta_{j} - \theta_{k} ) \right ) \\ J_{jj}^{P \theta} &= \frac{\partial P_{j}(\vec{x})}{\partial \theta_{j}} = -Q_{j} (\vec{x} ) - B_{jj} \vert V_{j} \vert ^{2} \\ J_{jk}^{Q \theta} &= \frac{\partial Q_{j}(\vec{x})}{\partial \theta_{k}} = - \vert V_{j} \vert \vert V_{k} \vert \left ( G_{jk} cos(\theta_{j} - \theta_{k}) + B_{jk} sin(\theta_{j} - \theta_{k}) \right ) \\ J_{jj}^{Q \theta} &= \frac{\partial Q_{j}(\vec{x})}{\partial \theta_{k}} = P_{j} (\vec{x} ) - G_{jj} \vert V_{j} \vert ^{2} \\ J_{jk}^{PV} &= \frac{\partial P_{j} (\vec{x} ) } {\partial \vert V_{k} \vert } = \vert V_{j} \vert \left ( G_{jk} cos(\theta_{j} - \theta_{k}) + B_{jk} sin(\theta_{j} - \theta_{k}) \right ) \\ J_{jj}^{PV} &= \frac{\partial P_{j}(\vec{x})}{\partial \vert V_{j} \vert } = \frac{P_{j} (\vec{x} )}{\vert V_{j} \vert} + G_{jj} \vert V_{j} \vert \\ J_{jk}^{QV} &= \frac{\partial Q_{j} (\vec{x} ) } {\partial \vert V_{k} \vert } = \vert V_{j} \vert \left ( G_{jk} sin(\theta_{j} - \theta_{k}) + B_{jk} cos(\theta_{j} - \theta_{k}) \right ) \\ J_{jj}^{QV} &= \frac{\partial Q_{j}(\vec{x})}{\partial \vert V_{j} \vert } = \frac{Q_{j} (\vec{x} )}{\vert V_{j} \vert} - B_{jj} \vert V_{j} \vert \\ \end{align}

The linear system of equations that is solved in every Newton iteration can be written in matrix form as follows:

\begin{align} -\left [ \begin{array}{cccccc} \frac{\partial \Delta P_{2} }{\partial \theta_{2}} & \cdots & \frac{\partial \Delta P_{2} }{\partial \theta_{N}} & \frac{\partial \Delta P_{2} }{\partial \vert V_{N_{G+1}} \vert} & \cdots & \frac{\partial \Delta P_{2} }{\partial \vert V_{N} \vert} \\ \vdots & \ddots & \vdots & \vdots & \ddots & \vdots \\ \frac{\partial \Delta P_{N} }{\partial \theta_{2}} & \cdots & \frac{\partial \Delta P_{N}}{\partial \theta_{N}} & \frac{\partial \Delta P_{N}}{\partial \vert V_{N_{G+1}} \vert } & \cdots & \frac{\partial \Delta P_{N}}{\partial \vert V_{N} \vert} \\ \frac{\partial \Delta Q_{N_{G+1}} }{\partial \theta_{2}} & \cdots & \frac{\partial \Delta Q_{N_{G+1}} }{\partial \theta_{N}} & \frac{\partial \Delta Q_{N_{G+1}} }{\partial \vert V_{N_{G+1}} \vert } & \cdots & \frac{\partial \Delta Q_{N_{G+1}} }{\partial \vert V_{N} \vert} \\ \vdots & \ddots & \vdots & \vdots & \ddots & \vdots \\ \frac{\partial \Delta Q_{N}}{\partial \theta_{2}} & \cdots & \frac{\partial \Delta Q_{N}}{\partial \theta_{N}} & \frac{\partial \Delta Q_{N}}{\partial \vert V_{N_{G+1}} \vert } & \cdots & \frac{\partial \Delta Q_{N}}{\partial \vert V_{N} \vert} \end{array} \right ] \left [ \begin{array}{c} \Delta \theta_{2} \\ \vdots \\ \Delta \theta_{N} \\ \Delta \vert V_{N_{G+1}} \vert \\ \vdots \\ \Delta \vert V_{N} \vert \end{array} \right ] = \left [ \begin{array}{c} \Delta P_{2} \\ \vdots \\ \Delta P_{N} \\ \Delta Q_{N_{G+1}} \\ \vdots \\ \Delta Q_{N} \end{array} \right ] \end{align}

Solution of the Problem

The solution update formula is given by:

\begin{align} \vec{x}^{(i+1)} = \vec{x}^{(i)} + \Delta \vec{x}^{(i)} = \vec{x}^{(i)} - \textbf{J}^{-1} \vec{f} (\vec{x}^{(i)}) \end{align}

To sum up, the NR algorithm, for application to the power flow problem is:

Set the iteration counter to $i=1$ . Use the initial solution $V_{i} = 1 \angle 0^{\circ}$
Compute the mismatch vector $\vec{f}({\vec{x}})$ using the power flow equations
Perform the following stopping criterion tests:
- If $\vert \Delta P_{i} \vert < \epsilon_{P}$ for all type PQ and PV buses and
- If $\vert \Delta Q_{i} \vert < \epsilon_{Q}$ for all type PQ
- Then go to step 6
- Otherwise, go to step 4.
Evaluate the Jacobian matrix $\textbf{J}^{(i)}$ and compute $\Delta \vec{x}^{(i)}$ .
Compute the update solution vector $\vec{x}^{(i+1)}$ . Return to step 3.
Stop.

Last modified 04.04.2025: Allow builds without nlohmann/json library (#362) (839af1a)